WEBVTT

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Anna: Welcome to Astronomy Daily. I'm Anna. And

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today we'll start with the exciting news of a

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new interstellar visitor. Only the third ever

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confirmed to be zooming through our solar

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system. Then we'll explore NASA's

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SphereX mission which is creating an all sky

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map of the universe, making its data

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publicly accessible. Next,

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prepare for a mind bending story about a self

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destructive exoplanet. An astonishing

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discovery. We'll also dive into the latest

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revelations from the James Webb Space

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Telescope, which continues to reshape our

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view of cosmic history. And finally, we'll

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uncover a surprising twist how Earth's

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very own weather satellites are now helping

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us study Venus.

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Let's get started. Our first

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stop today is an exciting new celestial

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visitor. Astronomers have just confirmed the

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discovery of an interstellar object, space

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speeding through our solar system. This marks

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only the third time humanity has detected an

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object that originated beyond our own stellar

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neighbourhood. The Visitor, officially

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named 3i Atlas by the International

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Astronomical Union's Minor Planet Centre, has

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been classified as a comet. Its

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fuzziness, as described by astronomer

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Jonathan McDowell from the Harvard

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Smithsonian Centre for Astrophysics, suggests

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it's primarily made of ice rather than rock.

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While its exact size is still being refined,

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current estimates place it at roughly 10 to

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20 kilometres wide, which would make it the

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largest interstellar interloper ever

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detected. However, if it's truly made of ice,

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it could be smaller since ice reflects more

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light, making it appear larger.

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Regardless of its precise dimensions, it

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poses absolutely no threat to Earth.

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Richard Moisel, head of Planetary defence at

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the European Space Agency, assures us it will

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fly deep through our solar system, passing

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just inside the orbit of Mars without any

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collision risk. What makes 3i

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Atlas so fascinating is its incredible speed.

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Zooming along at more than 60 kilometres per

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second, or about 37 miles per second,

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this phenomenal velocity means it isn't

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gravitationally bound by the sun. Unlike

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comets and asteroids that originate from

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within our solar system, its trajectory

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clearly indicates it's from interstellar

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space and will continue on its journey back

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out into the galaxy once it passes us.

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Astronomers theorise that these icy wanderers

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form around other star systems. As another

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star passes nearby, its gravitational tug can

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free these ice balls, sending them rogue into

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the galaxy. This newly discovered comet is

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simply one that happens to be passing through

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our cosmic backyard. The object

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was initially spotted by the NASA funded

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ATLAS survey in Hawaii. Professional and

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amateur astronomers worldwide then joined

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forces, digging through past telescope data

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to trace its path back to at least mid June.

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It's expected to get brighter and closer to

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the sun until late October and will remain

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observable by telescope into next year.

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To put this discovery into perspective, the

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first interstellar object, Oumuamua,

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was detected in 2017 and was so

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peculiar it even led some scientists to

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speculate about alien origins, though this

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theory has since been largely dismissed. Our

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second visitor, 2i Borisov, was

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observed in 2019. Mark Norris, an

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astronomer at the University of Central

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Lancashire in the UK, notes that 3i

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Atlas appears to be moving considerably

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faster than its two predecessors. While it's

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currently roughly the distance of Jupiter

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away from Earth and primarily visible in the

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southern hemisphere, its presence is

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incredibly significant. Scientists

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estimate that as many as 10,000 interstellar

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objects might be drifting through our solar

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system at any given time, though most are

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likely much smaller. This new detection

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suggests that observatories like the newly

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online Vera C Rubin Observatory in Chile

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could soon be finding these dim interstellar

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visitors on a monthly basis.

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Unfortunately, sending a mission to intercept

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3i Atlas isn't feasible due to its speed and

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trajectory. However, these rare

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visitors offer scientists an unparalleled

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opportunity to study material from outside

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our solar system. Imagine if we could detect

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precursors of life like, um, amino acids on

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such an object. It would give us immense

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confidence that the conditions for life exist

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in other star systems across the universe.

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Moving from interstellar visitors to an

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ambitious new mission let's talk about NASA's

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Sphere X telescope. Launched in March

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and now comfortably settled into low Earth

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orbit, this new Astrophysics space telescope

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has embarked on an incredible to create a

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comprehensive all sky map of the universe.

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What's truly revolutionary is that SphereX,

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which stands for Spectro Photometer for the

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History of the Universe, Epoch of

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Reionization and ICES Explorer has already

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begun delivering its sky survey data to a

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public archive on a weekly basis. This

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means anyone from professional astronomers to

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curious enthusiasts can access and use this

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data to unravel the universe's secrets.

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As Rachel Akcsson, the lead for the SphereX

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Science Data Centre, puts it, because we're

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looking at everything in the whole sky,

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almost every area of astronomy can be

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addressed by SphereX data. While other

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missions like NASA's retired WISE telescope,

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also mapped the entire sky, Sphere X

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significantly builds on that legacy. It

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observes in an astounding 102 infrared

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wavelengths, a massive leap compared to

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WISE's four wavelength bands. This extensive

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range allows scientists to use a technique

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called spectroscopy to identify the unique

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signatures of specific molecules. The

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mission's science team will harness this

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capability to study the distribution of

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frozen water and organic molecules, often

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referred to as the building blocks of life.

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According to across our own Milky Way galaxy

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beyond our cosmic neighbourhood. Sphere X

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data will be crucial for understanding the

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physics that drove the universe's rapid

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expansion after the Big Bang. It will also

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measure the amount of light emitted by all

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galaxies over cosmic time. The decision

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to make this data publicly available so

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quickly, within 60 days of collection is a

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testament to NASA's commitment to open

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science, transparency and efficiency. It

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empowers the entire astronomy community to

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explore and make discoveries that the Sphere

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X team alone couldn't possibly achieve.

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During its two year primary mission, SphereX

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will survey the entire sky twice a year,

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ultimately compiling four complete all sky

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maps. After the one year mark, a full map

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covering all 102 wavelengths will be

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released. The impact of SPHEREx extends

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even further as its data can be combined with

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observations from other groundbreaking

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missions. Imagine refining

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exoplanet parameters collected by NASA's

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Tess, identifying fascinating new targets for

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the James Webb Space Telescope, or studying

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the properties of dark matter and dark energy

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alongside the European Space Agency's Euclid

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mission and NASA's Nancy Grace Roman Space

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Telescope. The possibilities are truly

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boundless. As Vandana Desai, RSS

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Science Lead, wisely states, people are going

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to use the data in all kinds of ways that we

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can't imagine. It's an exciting time when the

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universe is becoming more accessible than

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ever, thanks to missions like SphereX, paving

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the way for unprecedented discoveries

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from the vast universe to individual

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planetary systems.

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Our next story takes us to a truly bizarre

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discovery, an exoplanet that seems to be

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actively contributing to its own demise.

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Astronomers have found a doomed planet

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officially named HIP67

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522B, which is clinging so tightly

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to its parent star that it's triggering

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explosive outbursts and in turn destroying

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itself. This is a completely new phenomenon

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in our understanding of celestial bodies. HIP

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67522B is a young

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extrasolar planet orbiting an equally young

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star, hip 67522, which

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is only about 17 million years old. To put

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that into perspective, our sun is a middle

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aged 4.6 billion years old. The

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exoplanet's orbit is incredibly tight,

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completing a full year in just one Earth

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week. Since the first exoplanets were

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discovered in the mid-1990s, scientists have

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wondered if a planet could orbit close enough

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to impact its star's magnetic fields. With

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over 5,000 exoplanet discoveries since then,

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the answer remained elusive. Until now.

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Ekaterina Ilien, the team leader from the

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Netherlands Institute for Radio Astronomy,

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expressed her excitement and curiosity,

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stating that they had never seen a system

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like HIP 67522B before,

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especially one with such a young planet

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orbiting so closely. She added that she had a

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million questions because the details of this

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new phenomenon are still unclear.

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The team first identified HIP

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67522B while using

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NASA's Transiting Exoplanet Survey Satellite,

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or TESS, which is designed to hunt for

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exoplanets and survey flaring stars.

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TESS picked up some intriguing

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characteristics, prompting a follow up

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investigation with the European Space

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Agency's Characterising Exoplanet Satellite,

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or cheops. With cheops, they observed even

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more flares, with almost all of them directed

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towards Earth as the planet passed in front

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of its star. What they discovered was

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remarkable. The stellar flares thrown out by

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hip 67522 occur

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precisely when its clingy planet transits or

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passes in front of the star. This

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strongly suggests that the flares are

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triggered by the planet itself. The leading

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theory is that hip

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67522B is so

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close to its star that it exerts a

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significant magnetic influence. As the planet

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whips around, it gathers energy, which is

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then redirected as waves rippling down the

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star's magnetic field lines. When one of

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these waves hits the stellar surface, it

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triggers a massive flare. Ilan

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explained that the waves seem to be setting

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off explosions that are in essence waiting to

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happen, resulting in flares with much higher

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energy than the waves themselves. This

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groundbreaking finding provides the first

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hard evidence that planets can indeed

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influence the behaviour of their stars. And

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for hip 67522B, this

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influence is disastrous. The induced flares

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are directed right back at the planet,

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bombarding it with approximately six times

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the radiation a planet at this orbital

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distance would typically experience.

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Currently, hip 67522B is

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about the size of Jupiter, but its density is

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incredibly low, comparable to candy floss.

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This intense radiation bombardment is

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stripping away the planet's wispy outer

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layers, causing it to lose what little mass

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it possesses over the next hundred million

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years. Circumstances scientists predict that

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hip 67522B could shrink from

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its current Jupiter like size to something

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closer to Neptune. The full extent of the

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damage from these self inflicted flares is

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still uncertain. But this bizarre celestial

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dance is opening up entirely new avenues for

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understanding star planet interactions and

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planetary evolution.

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Next up, let's take a look at an anniversary

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of sorts. Since July 2022,

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NASA's James Webb Space Telescope has been

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diligently focused on unlocking the

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universe's secrets. And it has absolutely

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delivered with its unparalleled ability to

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detect and analyse invisible infrared light.

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Webb has made observations once thought

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impossible, profoundly changing our view of

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the cosmos from the most distant galaxies

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to the familiar corners of our own solar

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system. Webb was built with the promise of

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revolutionising astronomy and rewriting the

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textbooks. And by any measure, it has far

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exceeded those lofty expectations. In

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just three years of science operations, Webb

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has completed more than 860 scientific

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programmes, collecting nearly 550

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terabytes of data and leading to over

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1600 research papers. The

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sheer volume of intriguing results and new

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questions it has raised is truly astonishing.

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One of Webb's primary missions was to observe

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cosmic dawn, the period during the universe's

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first billion years when the earliest stars

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and galaxies were forming. What scientists

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expected to see were a few faint, nascent

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galaxies, mere hints of what would eventually

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become the grand structures we see today.

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Instead, Webb revealed surprisingly bright

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and mature galaxies that developed within a,

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uh, mere 300 million years of the Big Bang.

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It also found galaxies with black holes that

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seemed far too massive for their age, and

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even an infant Milky Way type galaxy that

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existed when the universe was only 600

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million years old. This

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suggests that the universe evolves

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significantly faster than we previously

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thought. Adding to the surprises,

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Webb has unveiled a new type of galaxy. A

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distant population of mysteriously compact

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bright red galaxies, affectionately dubbed

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little red dots. What makes them so bright

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and red? Are they illuminated by dense

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groupings of unusually brilliant stars? By

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gas spiralling into a supermassive black

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hole? Or perhaps both. And what

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eventually happened to them? These little red

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dots appeared around 600 million years after

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the Big Bang and rapidly declined in number

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less than a billion years later, leaving

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astronomers eager to understand their

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evolution. Webb's observations are also

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providing critical insights into one of

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astronomy's most perplexing dilemmas the

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Hubble tension. This refers to the

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frustrating problem where different methods

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of calculating the universe's current

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expansion rate yield different results. Is it

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simply a matter of measurement errors? Or is

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there something truly strange happening in

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the cosmos? So far, Webb's data

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indicates that the Hubble tension is not due

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to measurement inaccuracies. By

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precisely distinguishing pulsating stars in

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crowded fields, and even discovering a

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distant gravitationally lensed supernova

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whose image appeared at three different times

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during its explosion, Webb is providing

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independent checks on these crucial

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measurements, suggesting this cosmic puzzle

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is very real.

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Beyond galaxies, the Webb telescope's

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extraordinary infrared vision has also

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unveiled surprisingly rich and varied

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atmospheres on gas giants orbiting distant

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stars. While the Hubble Space Telescope

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made the first detection of gases on an

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exoplanet, Webb has taken these studies to an

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entirely new level. It's revealed a chemical

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cocktail including hydrogen sulphide,

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ammonia, carbon dioxide, methane

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and sulphur dioxide, none of which had been

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clearly detected in an atmosphere outside our

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solar system before. Webb has even examined

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the exotic climates of these gas giants,

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detecting flakes of silica, uh, snow in the

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skies of one searing hot world and measuring

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temperature and cloud differences across

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others. The telescope's exceptional ability

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to measure subtle changes in infrared light

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makes it possible to even analyse the thin

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layers of gas around smaller rocky planets.

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Webb has already ruled out significant

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atmospheres on some rocky worlds and found

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tantalising signs of carbon monoxide or

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carbon dioxide on 55 Cancri E A, uh,

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lava world orbiting a sun like star. These

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findings are laying crucial groundwork for

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NASA's future habitable worlds Observatory,

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which will be designed to directly image and

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search for life on Earth. Like planets.

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Webb has also mapped intricate galaxy

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structures with unprecedented detail, showing

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us cosmic cities where stars form, live,

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die and are recycled into the next

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generation. Its infrared eyes reveal

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delicate filaments of dust tracing spiral

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arms, ancient star clusters forming galactic

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cores, newly forming stars still hidden in

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glowing cocoons of dust and gas, and clusters

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of hot young stars carving enormous cavities

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within the dust. It's truly helping us

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understand how stellar winds and explosions

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actively reshape their galactic homes.

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In other observations, Webb has spotted

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hundreds of objects resembling brown dwarfs

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in the Milky Way and even some candidates in

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a neighbouring galaxy. Brown dwarfs form like

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stars, but aren't massive enough to fuse

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hydrogen. Some of these objects are so small,

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just a few times the mass of Jupiter, that

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it's hard to tell if they're free floating

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gas giant planets or something else entirely.

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Thanks to Webb, we now know there's a

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continuous spectrum of objects ranging from

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planets to brown dwarfs to full fledged

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stars. The telescope has also found potential

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planets orbiting white dwarfs, hinting that

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it might be possible for worlds to survive

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the dramatic death of their host stars.

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Closer to home, Webb has turned its gaze to

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our own solar system with equally impressive

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results. It observed the vast water plume

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00:16:46.700 --> 00:16:49.020
erupting from Saturn's moon Enceladus,

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00:16:49.180 --> 00:16:51.820
revealing its true scale as a cloud spanning

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over 6,000 miles, about 20 times wider

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than Enceladus itself. This water then

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spreads out into a donut shaped torus

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encircling Saturn, even raining down onto the

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planet. The these unique observations of

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rings, auroras, clouds, winds,

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ices and gases are helping us better

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00:17:10.950 --> 00:17:12.990
understand what our cosmic neighbourhood is

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made of and how it has changed over time.

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Finally, Webb has also played a crucial role

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in Supporting asteroid defence missions. In

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2024, when an asteroid was discovered with a

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preliminary chance of hitting Earth, Webb was

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uniquely able to measure the object, which

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turned out to be the size of a 15 story

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building, helping assess the hazard. While

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that particular asteroid is no longer a

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threat, the study demonstrated Webb's

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capabilities. The telescope also provided

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vital support for NASA's Double Asteroid

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Redirection Test, or DART, mission, which

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deliberately impacted the Didymos binary

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asteroid system. Both Webb and Hubble

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observed the impact, confirming that the

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composition of these asteroids is typical of

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those that could threaten Earth. In just

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three years, Webb has brought the distant

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universe into sharp focus, revealed

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unexpectedly bright and numerous galaxies,

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unveiled new stars in their dusty cocoons,

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and studied weather on exoplanets. This is

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only the beginning. As engineers estimate

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Webb has enough fuel to continue observing

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for at least 20 more years, promising many

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more cosmic surprises to come.

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Finally, today, in a truly unexpected turn of

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events, Japanese meteorological satellites,

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the Himawari 8 and 9, which are typically

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used for monitoring Earth's global weather

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patterns, are now providing incredibly

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valuable insights into Venus's atmosphere.

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These satellites, launched in 2014

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and 2016 by the Japan

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Meteorological Agency, are equipped with

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multispectral advanced Himawari imagers.

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In a recent study led by the University of

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Tokyo in infrared, images from these

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satellites captured changes in Venus's

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atmosphere, revealing previously unseen

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temperature patterns in its cloud tops. This

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is a significant development because

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meteorological satellites can complement

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observations of Venus's atmosphere, which

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usually come from robotic missions and ground

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based telescopes. Scientists have been

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studying Venus's atmosphere for decades to

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understand the dynamics of our solar system's

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hottest planet. However, many

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mysteries persist, such as its thermal tides

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and planetary scale waves. Dedicated

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robotic probes have often been limited to

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single band imagery or short observation

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periods. That's where the Himawari satellites

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come in. Because these satellites are

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scheduled to remain operational for more than

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a decade, they offer an unprecedented

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opportunity for long term multi band

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monitoring. Their instruments provide

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infrared coverage that measures Venus's

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temperature across different bands, showing

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temporal variations. When these geostationary

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satellites align with Earth and Venus, they

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can obtain images of Venus's turbulent

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atmosphere, helping to fill crucial

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observational gaps. The team behind the

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study used hundreds of images from Himawari 8

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and 9 to map the temporal dynamics and track

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temperature variations in Venus's cloud tops

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over time. Their analysis confirmed that both

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the thermal tides and planetary waves in

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Venus's atmosphere are subject to changes in

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amplitude over time, which decrease with

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altitude. This novel approach opens

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new avenues for long term and multiband

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monitoring of other solar system bodies,

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including the Moon and Mercury. By

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providing continuous data that dedicated

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missions might miss due to their shorter

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lifespans, these Earth focused satellites are

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unexpectedly contributing to our broader

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understanding of planetary evolution.

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That's all for this episode of Astronomy

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Daily. I'm Anna and I hope you enjoyed our

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00:20:43.300 --> 00:20:45.440
journey through the latest in space and

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00:20:45.440 --> 00:20:48.280
astronomy news. Thank you for tuning in. If

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00:20:48.280 --> 00:20:50.280
you want to catch up on all the latest space

501
00:20:50.280 --> 00:20:52.200
and astronomy news with our constantly

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00:20:52.200 --> 00:20:54.080
updating newsfeed, or listen to all our back

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episodes, be sure to visit our website at

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astronomydaily IO. You can also stay

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connected with us on social media. Just

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and TikTok for daily updates and more cosmic

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content. Until next time, keep looking up and

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00:21:11.610 --> 00:21:12.250
stay curious.
